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Abundances of Solar Cosmic Ray Protons and Alpha Particles for 1969-1972

✍ Scribed by Stroscio, Michael A.; Katz, Ludwig; Yates, G. Kenneth; Sellers, Bach; Hanser, Frederick A.

Book ID
119712181
Publisher
American Geophysical Union
Year
1976
Tongue
English
Weight
401 KB
Volume
81
Category
Article
ISSN
0148-0227

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πŸ“œ SIMILAR VOLUMES

The acceleration and propagation of sola
The acceleration and propagation of solar cosmic rays as deduced from the relative abundance of protons to helium nuclei
✍ Kunitomo Sakurai πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 488 KB

Except for protons, the chemical composition of solar cosmic rays is very similar to the abundance of the elements at the photosphere of the Sun. If we consider the relative abundance ratio of protons to a-particles (P/a) at constant rigidity, this ratio is highly variable from one solar cosmic ray

Variations of the relative abundances of
Variations of the relative abundances of He, (C, N, O) and Fe-group nuclei in solar cosmic rays and their relationship to solar particle acceleration
✍ D. L. Bertsch; S. Biswas; C. E. Fichtel; C. J. Pellerin; D. V. Reames πŸ“‚ Article πŸ“… 1973 πŸ› Springer 🌐 English βš– 638 KB

Measurements of the flux of helium nuclei in the 24 January, 1971, event and of helium and (C, N, O) nuclei in the 1 September, 1971, event are combined with previous measurements to obtain the relative abundances of helium, (C, N, O), and Fe-group nuclei in these events. These data are then summari